Published October 15, 1975
| Version v1
Journal article
Neutrino magnetic moment, plasmon Cerenkov radiation, and the solar-neutrino problem
Description
Clark and Pedigo suggested that, if the neutrino has a magnetic moment, the energy loss of a solar neutrino in escaping the sun, due to magnetic elastic scattering off electrons, could help explain the absence of detection of solar neutrinos at earth. Collective effects of the solar plasma will modify the energy loss calculated by those authors. The existence of the possibility of Cerenkov radiation of longitudinal plasmons suggests that the effect might be large and positive. Detailed calculation shows that it is actually a small effect on the energy loss and not of likely impact on the solar-neutrino problem
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review D
- Journal Volume
- 12
- Journal Issue
- 8
- Series
- Phys. Rev., D.
- Journal Page Range
- 2208-2211
- ISSN
- 0556-2821
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 7247386
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- ENERGETIC SOLAR PARTICLES; ENERGY LOSSES; FOURIER TRANSFORMATION; MAGNETIC MOMENTS; NEUTRINO-ELECTRON INTERACTIONS; NEUTRINOS; PLASMONS; SOLAR RADIATION
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; INTEGRAL TRANSFORMATIONS; INTERACTIONS; LEPTON-LEPTON INTERACTIONS; LEPTONS; MASSLESS PARTICLES; PARTICLE INTERACTIONS; QUASI PARTICLES; RADIATIONS; STELLAR RADIATION; TRANSFORMATIONS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent